On the degeneracy between w 0 and w a Yungui Gong Huazhong Univ of Science and Tech 华中科技大学 龚云贵 The 7 th Aegean Summer School, Paros, Greece,
Contents Motivations: General Property of Scalar Field dynamics Dark energy parametrizations The degeneracy between w 0 and w a The consequence of the derived degeneracy
Motivations General Property of scalar field dynamics scalar field as dark energy: Tracking solutions Tracker fields (Steinhardt etal, PRD 1999)
Tracking Solutions
Tracking Solution: General Property Almost independent of initial conditions Relation Common Dynamics for scalar fields
Efstathiou Parametrization Dark energy parametrization: capture the main dynamics of scalar field MNRAS 383, 879 (1999)
CPL Parametrization Approximation E. Linder astro-ph/
The degeneracy in CPL model w 0 and w a is degenerated What is the degeneracy? related with ?
Dark Energy Parametrizations (Partial Lists) Dark energy parametrization: capture the main dynamics of scalar field Efstathiou 1999, MNRAS 310, 842 CPL, Chevallier & Polarski 2001, IJMPD 10, 213; Linder 2003, PRL 90, JBP, Jassal, Bagla & Padmanabhan, MNRAS 356, L11 Wetterich 2004, PLB 594, 17
Scalar Field approximation Cosmological equations
Scalar Field Dynamics Take the (Slow-roll) approximation For Thawing scalar field Scherrer & Sen 2008, PRD 77,
approximation
Thawing scalar fields Approximate w(z) dotted curve short dash curve long dash curve
The degeneracy between and Relation 0 th order approximation Scherrer and Sen 2008, PRD 78,
SSLCPL model Taylor Expansion Gong etal., Int. J. Mod. Phys. 22 (2013) ,
The accuracy of the approximation
SSWCPL model Take approximation
The accuracy of the approximation
The degeneracy Self-consistency
Flat SSLCPL Results
Flat SSWCPL Results
Flat CPL Results
Comparisons
Conclusions The dynamics of scalar fields has some common features The exists an approximate relation between w and For thawing models, the dynamics can be approximated by CPL parametrization with degenerated relation between w 0 and w a The reduced degeneracy helps improve the constraint on w(z)
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